IPs
AE Aqr
FO Aqr
XY Ari
V405 Aur
HT Cam
MU Cam
DW Cnc
BG CMi
V709 Cas
V1025 Cen
TV Col
TX Col
UU Col
V2069 Cyg
V2306 Cyg
YY Dra
PQ Gem
DQ Her
EX Hya
NY Lup
V2400 Oph
GK Per
AO Psc
WX Pyx
V1223 Sgr
V1062 Tau
EI UMa
IGR 00234
IGR 15094
IGR 17303
Swift J0732
RX J0704
RX J1803
RX J2133
SDSS J233325
XSS 00564
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DQ Herculis = Nova Herculis 1934

SkyView image
of DQ Her (see important notes)
- Position
-
- Equatorial: 18h07m30.12s,
+45d51m32.7s (J2000)
- Galactic: l=73.15, b=+26.44
- Finding Chart:
-
- Brigntness:
- Optical ; fx (2-10 keV)~?
- IP Credential:
- ***** (Confirmed)
- Periods:
-
- Orbital: 0.19362 d = 4.65 hr = 16729 s, from optical eclipses.
Tmin = HEJD 2434954.94429(8) + 0.1936208964(12)E
(Zhang et al. 1995,
who also give a quadratic version).
- Spin: 8.2252e-02 day = 1.18 min = 71.066 s, seen in optical photometry.
Tmax = HEJD 2439628.77177(3) + 8.22518320(3)e-04 E
- 2.62(4)e-16 E^2 + 2.8(1)e-24 E^3
(Zhang et al. 1995).
The 71 s period has long been thought to be the spin period, but
Zhang et al. 1995 prsents
strong (but indirect) evidence that the true spin period is twice this value.
- Others:
- Inclination:
- ~90 deg (deep eclipse, front half of disk is probably hidden)
- Distance:
- 525+/-28 pc (Vaytet, O'Brien & Rushton 2007;
see also Herbig & Smak 1992,
who obtained 561+/-19 pc)
References
We will not even attempt to compile a complete list of pre-1980 papers
that deal exclusively with the classical nova event of 1934; see the
Bode and Evans book on Classical Novae for that.
Please send your comments, suggestions etc. to
Koji.Mukai@nasa.gov
and/or
Koji.Mukai@umbc.edu
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